'Sz effect' presentation slideshows

OLIMPO

(http://oberon.roma1.infn.it/olimpo). OLIMPO. An arcmin-resolution survey of the sky at mm and sub-mm wavelengths. Silvia Masi Dipartimento di Fisica La Sapienza, Roma and the OLIMPO team. (http://oberon.roma1.infn.it/olimpo). OLIMPO. An arcmin-resolution survey of the sky

904 views • 70 slides

The microwave background radiation and the Sunyaev-Zel’dovich effect

The microwave background radiation and the Sunyaev-Zel’dovich effect. Mark Birkinshaw. Outline. The microwave background The origin of the SZ effect SZ observations today Cluster structures and SZ effects Cosmology and SZ effects AMiBA and OCRA Summary. 1. The microwave background.

795 views • 63 slides

636 views • 63 slides

657 views • 57 slides

Relativistic Corrections to the Sunyaev-Zeldovich Effect for Clusters of Galaxies

Carolina Neutrino Workshop April 16-17th, 2004. 1/33. Relativistic Corrections to the Sunyaev-Zeldovich Effect for Clusters of Galaxies. Satoshi Nozawa Josai Junior College for Women. Collaborators: N. Itoh, Y. Kohyama. 2/33. Contents.

346 views • 34 slides

Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School

Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School. 1. Unidentified CMB signal (T.Shmaonov, 1957, Ph.D) 2. CMB or Black Body population of Radio Sources? (Y.Par, 1968) 3.CMB polarization (Penzias: <100mK; Pulkovo: <1mK)

424 views • 31 slides

The SZ effect: Surveys and Cosmology

The SZ effect: Surveys and Cosmology. Michele Limon Columbia University. Structure Formation. Standard ? CDM Model Box Size 43 Mpc 3 30 > z > 0. In typical structure formation scenarios, low mass clusters emerge in significant numbers at z~2-3.

466 views • 30 slides

SZ effect and ALMA workshops

276 views • 27 slides

ALMA/ARC 2007 March 2, 2007

ALMA/ARC 2007 March 2, 2007. Astro Particle Cosmology. Studying SZ Effect s with ALMA. Sergio Colafrancesco INAF - Osservatorio Astronomico di Roma Email : Sergio.C olafrancesco@mporzio.astro.it. SZ effect: the standard lore. I 0 (x). I(x). thermal NR e -.

365 views • 26 slides

Galaxy clusters are the most massive (M~10 14 -10 15 M SUN ) objects in the Universe

The astrophysics of galaxy clusters: from X- rays to SZ effect (Part I) Mariachiara Rossetti Milano, 04 /04/ 2012. GALAXY CLUSTERS:WHAT?. Intra-cluster medium (ICM) X-rays (10-30%). Galaxies (5%). Dark Matter Gravitational potential. 1E 0657-156 THE BULLET CLUSTER.

255 views • 25 slides

Using the Sunyaev-Zeldovich Effect to Determine H o and the Baryon Fraction

361 views • 23 slides

SZ Surveys Are Coming: What should we do?

233 views • 23 slides

Measurements of Cosmological Parameters

301 views • 21 slides

A self-similar study of SZ cluster number counts from X-ray properties

290 views • 20 slides

Zheng , Yi ?? Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y. Zheng , 1207.2722.

Peculiar velocity decomposition, redshift distortion and velocity reconstruction in redshift surveys. Zheng , Yi ?? Shanghai Astronomical Observatory P . Zhang, J. Pan, and Y. Zheng , 1207.2722. Y. Zheng , P. Zhang et al. (2012), in preparation. Outline .

334 views • 12 slides

SZ effect

Observing the SZ Effect with the IRAM 30-meter and the Plateau de Bure Interferometer (on behalf of Francois-Xavier Desert). SZ effect. Diffraction is 18" at 2 mm. - High resolution measurements - Complement to X-ray data (XMM-Newton, Chandra, Rosat) and the future Planck. Diabolo cryostat

333 views • 12 slides

SZ effect

Observing the SZ Effect with the IRAM 30-meter and the Plateau de Bure Interferometer (on behalf of Francois-Xavier Desert). SZ effect. Diffraction is 18" at 2 mm. - High resolution measurements - Complement to X-ray data (XMM-Newton, Chandra, Rosat) and the future Planck. Diabolo cryostat

257 views • 12 slides